Gravitational waves in non-singular string cosmologies

DOI10.1016/S0550-3213(01)00182-1zbMath0969.83549arXivgr-qc/0101019WikidataQ63391144 ScholiaQ63391144MaRDI QIDQ5940099

Cyril Cartier, Edmund J. Copeland, M. Gasperini

Publication date: 25 July 2001

Published in: Nuclear Physics. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/gr-qc/0101019

zbMATH Keywords

higher-order correctionsstring effective actiontensor metric fluctuations

Mathematics Subject Classification ID

Relativistic cosmology (83F05) String and superstring theories in gravitational theory (83E30) Geometrodynamics and the holographic principle (83E05) Gravitational waves (83C35)

Related Items (4)

Oscillation in power spectrum of primordial gravitational wave as a signature of higher-order stringy corrections ⋮ Anisotropic homogeneous string cosmology with two-loop corrections ⋮ Low-energy graceful exit in anisotropic string cosmology backgrounds ⋮ Density perturbations in the ekpyrotic Universe and string-inspired generalizations

Cites Work

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• Towards a non-singular pre-big bang cosmology
• Pre-big-bang bubbles from the gravitational instability of generic string vacua
• Quantum inhomogeneities in string cosmology
• Initial conditions and the structure of the singularity in pre-big-bang cosmology
• INFLATION, DEFLATION, AND FRAME-INDEPENDENCE IN STRING COSMOLOGY
• Sensitivity of a VIRGO pair to relic gravitational wave backgrounds
• Back Reaction and Graceful Exit in String Inflationary Cosmology
• Semiclassicality and decoherence of cosmological perturbations
• The graceful exit in pre-big bang string cosmology

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